The problem of heating the Sun's corona requires: (a) the conversion of magnetic energy into thermal energy and (b) a continuous heating theory. One of the most promising mechanisms for heating the solar corona is nanoflare heating along with avalanche effects. During the presentation, I will show a series of simulations showing how the relaxation process (Taylor 1974, 1986) may trigger energy release in nearby loops (Tam et al. 2015 and Hood et al., 2016).

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抚仙湖太阳观测与研究基地

云南天文台学术委员会

邀请人：抚仙湖研究基地，刘忠

12月5日